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NGC 4559 — Galaxy in Coma Berenices

Galaxy Excellent (64/100)

Spiral

Magnitude 9.9m Galaxy Coma Berenices (Com) Visible
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About NGC 4559

Description

NGC 4559 is a barred spiral galaxy in Coma Berenices, about 29 million light-years away. It is a loose, patchy spiral with numerous HII star-forming regions and appears roughly 10 arcminutes long with low surface brightness.

Observing Tips

Visible as a faint, elongated glow in a 6-inch telescope. Dark skies are important for this low-surface-brightness galaxy. Best viewed in spring evenings at low to medium magnification.

History

Discovered by William Herschel on April 11, 1785. X-ray observations have revealed an ultraluminous X-ray source in this galaxy that may be an intermediate-mass black hole.

Fun Facts

NGC 4559 contains an unusually large number of bright HII regions for its size, indicating vigorous ongoing star formation.

Observe

1Properties

Magnitude 9.9
Angular Size 10.6′ × 4.8′
Position Angle 148°
Distance 37.98 million ly
Galaxy Type Spiral (SABcd)
vB, vL, mE 150deg , gbM, 3 st f

Position & Identifiers

RA 12h 35m 57.6s
Dec +27° 57' 36.0"
Catalog NGC 4559

2How easy to spot?

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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Medium+ Medium Hard+
150mm Newt. Easy Easy Medium+
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

Easy on Seestar S50

3Visibility

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Best season Feb – Apr (peak: Mar)

4 Eyepiece View

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125x TFOV: 0.4° Lim. mag: 13.6
N E

NGC 4559 · 10.6′×4.8′ · N up, E left

5 Best Magnification

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6 Surface Brightness

7 Morphology Decoder

8 Inclination & True Shape

9 Redshift

10 Size Comparator

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11

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12

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